activity
20122021
most citedThe Comptonising medium of the neutron star in 4U 1636-53 through its lower kilohertz Quasi-Periodic Oscillations

97 citations · 341 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2021

X-ray emitting structures in the Vela SNR: ejecta anisotropies and progenitor stellar wind residuals

Vincenzo Sapienza, Marco Miceli, Giovanni Peres +6

The Vela supernova remnant (SNR) shows several ejecta fragments protruding beyond the forward shock (shrapnel). Recent studies have revealed high Si abundance in two shrapnel (A an…

astro-ph.HE202153 cited

A variable corona for GRS 1915+105

Konstantinos Karpouzas, Mariano Méndez, Federico García +4

Most models of the low frequency quasi periodic oscillations (QPOs) in low-mass X-ray binaries (LMXBs) explain the dynamical properties of those QPOs. On the other hand, in recent…

astro-ph.HE2021

Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario

Federico García, Adolfo Simaz Bunzel, Sylvain Chaty +2

We aim to study the progenitor properties and expected rates of the two lowest-mass binary black hole (BH) mergers, GW 151226 and GW 170608, detected within the first two Advanced…

astro-ph.HE20204 cited

Stellar wind structures in the eclipsing binary system IGR J18027-2016

Federico A. Fogantini, Federico García, Jorge A. Combi +1

IGR J18027-2016 is an obscured high-mass X-ray binary formed by a neutron star accreting from the wind of a supergiant companion with a 4.57 day orbital period. The source sh…

astro-ph.HE202087 cited

A two-component Comptonisation model for the type-B QPO in MAXI J1348-630

Federico García, Mariano Méndez, Konstantinos Karpouzas +3

Spectral-timing analysis of the fast variability observed in X-rays is a powerful tool to study the physical and geometrical properties of the accretion/ejection flows in black-hol…

astro-ph.HE201997 cited

The Comptonising medium of the neutron star in 4U 1636-53 through its lower kilohertz Quasi-Periodic Oscillations

Konstantinos Karpouzas, Mariano Méndez, Evandro M. Ribeiro +3

Inverse Compton scattering dominates the high energy part of the spectra of neutron star (NS) low mass X-ray binaries (LMXBs). It has been proposed that inverse Compton scattering…